Title: Nuclear%20Chemistry
1Nuclear Chemistry
2What makes a nucleus Stable?
- Must have a good ratio of protons and neutrons.
- This ratio is defined in a band of stability.
- There are other aspects that seem arbitrary.
- What?
3A plot of the stable nuclei reveals a band of
stability.Nuclei outside the band are unstable.
Positron emission
4Types of decay
- A stable nucleus must have the right combination
of protons and neutrons. - Too big Alpha decay
- Too many protons positron emission
- Too many neutrons Beta decay
- Nucleus has excess energy Gamma decay
5Beta Decay
- Occurs if there are too many neutrons.
- A neutron to proton conversion occurs. This
releases an electron or beta particle. - Carbon-14 undergoes beta decay to the stable
nitrogen-14 isotope.
6Balancing Nuclear Equations
- Sum of top numbers on the left must equal sum of
top numbers on right. - Same thing for bottom numbers.(Check the C-14
example)
Top 14140 Bottom 6 7-1
7Positron Emission
- Isotopes on the lower side of the band of
stability might want to turn a proton into a
neutron through positron emission. - A positron is essentially a positive electron.
Top 11110 Bottom 6 51
8Alpha Decay
- Large isotopes that need to decrease their size
tend to decay by alpha emission. - An alpha particle can be described as a helium
nucleus, , 2 protons and 2 neutrons.
9Uranium Decay
- A nuclear decay may not always produce a stable
isotope directly. - Uranium-238 undergoes 14 decays.
10 Gamma Decay (g)
- The gamma ray is not a particle it is part of the
electromagnetic spectrum. - Gamma radiation occurs when a nucleus has excess
energy. - Some nuclei can exist for a little while with
excess energy. These are called meta-stable
isotopes. Technetium 99 has a meta-stable
isotope. - A gamma ray can be represented by ?.
11Technetium-99 has a meta-stable isotope.
Top 9999 Bottom 43 43
Technetium-99 is used in medical applications.
Another link
12Fission and Fusion
- Nuclear Fission involves the breaking up of large
nuclei to smaller nuclei. link - Nuclear Fusion is the energy-producing process,
which takes place continuously in the sun and
stars. In the core of the sun at temperatures of
10-15 million degrees Celsius, Hydrogen is
converted to Helium providing enough energy to
sustain life on earth. link
13Nuclear fission of U-235
14Types of Radiation
Stopped by Damage to Cells
Alpha almost anything. example paper Most Damage
Beta wood, heavy clothing, plastic
Gamma lead, concrete Least Damage
15Protect yourself by
- Minimizing time of exposure
- Distance
- Shielding
lung
16Half Life
- The half-life of a radioisotope is the time it
takes for one half of a sample to decay. - Iodine-131 has a half-life of 8 days.
Days Amount of 131I
0 40
8 20
16 10
24 5
32 2.5
40 1.25
17The decay of an isotope is not linear.
18Carbon Dating
- An archeologist extracts a sample of carbon from
an ancient ax handle and finds that it emits an
average of 10 beta emissions per minute. She
finds that the same mass of carbon from a living
tree emits 40 beta particles per minute. - Knowing that the half life of carbon-14 is 5730
years, she concludes that the age of the ax
handle is?
19Measuring radiation
- Curie the amount of any radionuclide that
undergoes 37 billion atomic transformations a
second. - A nanocurie is one one-billionth of a curie.
- A Becquerel is one disintegration per second.
- 37 Becquerel, 1 nanocurie
- The curie is proportional to the number of
disintegrations per second.
20RAD
- Rad (radiation absorbed dose) measures the amount
of energy actually absorbed by a material, such
as human tissue - Takes into account the absorbing material. (Bone
may absorb better then skin or muscle).
21REM
- Rem (roentgen equivalent man) measures the
biological damage of radiation. - REMRADRBE
- RBE (relative biological effect) takes into
account that alpha particles are 10 X more
damaging than beta particles. - LD50 500 rems